Extrinsically flat static spacetimes

dc.creatorZaslavskii, O. B.
dc.date2006-04-21
dc.date.accessioned2026-07-07T07:09:39Z
dc.date.available2026-07-07T07:09:39Z
dc.descriptionWe consider static spacetimes whose spatial part admits foliations with the extrinsic curvature tensor K_{ab}=0. There are two complementary cases when the gradient of the lapse function points 1) to the direction of foliation or 2) orthogonally to it. Case 1) gives generalization of metrics like Bertotti-Robinson or Nariai. In case 2) the matter source violates the null energy condition at least on the part of the manifold, having in this sense phantom nature. We also demonstrate that for the manifolds under discussion the horizon can be naked in the sense that certain Weyl components diverge in the free-falling frame although the Kretschmann scalar is finite. The Petrov type is D or O. Explicit solutions for (i) the linear anisotropic equation of state, (ii) Chaplygin gas and (iii) uniform energy density are found.
dc.description25 pages. To appear in Class. Quant. Grav
dc.identifierhttps://arxiv.org/abs/gr-qc/0604097
dc.identifierhttp://arxiv.org/abs/gr-qc/0604097
dc.identifierClass.Quant.Grav. 23 (2006) 4083-4100
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111149
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.subjectDifferential Geometry
dc.titleExtrinsically flat static spacetimes
dc.typetext

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